Description |
We submit this DDT proposal to secure crucial SPIRE observations of a hitherto unexplored population of extremely mm-bright and radio-loud sources discovered by the South Pole Telescope (SPT). Only SPIRE observations can provide the adequate wavelength coverage (at 250, 350, and 500micron) to accurately constrain the spectral energy distributions of these radio-loud SPT sources, as well as their IR luminosities, dust temperatures, and redshift distribution. |